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- W2023084541 abstract "Abstract We alert the community to a paradigm method to calibrate a range of standard candles by means of well-calibrated photometry of eclipsing binaries in star clusters. In particular, we re-examine systems studied as part of our Binaries-in-Clusters program, and previously analyzed with earlier versions of the Wilson–Devinney light-curve modeling program. We make use of the 2010 version of this program, which incorporates a procedure to estimate the distance to an eclipsing system directly, as a system parameter, and is thus dependent on the data and analysis model alone. As such, the derived distance is accorded a standard error, independent of any additional assumptions or approximations that such analyses conventionally require." @default.
- W2023084541 created "2016-06-24" @default.
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- W2023084541 date "2012-08-01" @default.
- W2023084541 modified "2023-09-25" @default.
- W2023084541 title "Application of the Direct Distance Estimation procedure to eclipsing binaries in star clusters" @default.
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- W2023084541 doi "https://doi.org/10.1017/s174392131202145x" @default.
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